A bstract Kerr-Newman de Sitter (KNdS) spacetimes have a rich thermodynamic structure
that involves multiple horizons, and so differs in key respects from asymptotically flat or AdS …

This paper is devoted to study the thermodynamic topological defects, Joule–Thomson (J−
T) and Maxwell's equal area law of Phantom RN AdS black holes (BHs). The inversion …

From solving the equations of the motion for a system of Einstein gravity coupled to a non-
linear electromagnetic field in the dS spacetime with two integral constants, we derived a …

There exist several well-established procedures for computing thermodynamics for a single
horizon spacetime. However, for a spacetime with multi-horizon, the thermodynamics is not …

We investigate the thermodynamics of the Einstein-non linear-Maxwell-Yukawa black hole
solution in de Sitter spacetime. After presenting the black hole solution and its horizons, we …

The absence of a true thermodynamical equilibrium for an observer located in the causal
area of a Schwarzschild–de Sitter spacetime has repeatedly raised the question of the …

We consider a Schwarzschild–de Sitter (SdS) black hole, and focus on the emission of
massless scalar fields either minimally or non-minimally coupled to gravity. We use six …

The creation of a thermal distribution of particles by a black hole is independent of the detail
of gravitational collapse, making the construction of the eternal horizons sufficient to address …

On the basis of the state parameter of de Sitter space-time satisfying the first law of
thermodynamics, we can derive some effective thermodynamic quantities. When the …

The phase transition of the Einstein‐Gauss‐Bonnet AdS black hole has the similar property
with the van der Waals thermodynamic system. However, it is determined by the Gauss …